RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 7.0077e-04 Jy/beam
minimum 1.1602e-04 Jy/beam
mean 1.9993e-04 Jy/beam
median 1.4741e-04 Jy/beam
sigma 9.8611e-05 Jy/beam
MAD rms 2.3083e-05 Jy/beam

RMS images

VLASS2.1.sb38619750.eb38664746.59114.89728754629_split.ms

VLASS2.1.ql.T18t17.J120215_283000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T18t17.J120215+283000_P70818v1_2020_09_22T17_12_23.397/working/VLASS2.1.sb38619750.eb38664746.59114.89728754629_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T18t17.J120215+283000_P70818v1_2020_09_22T17_12_23.397/working
Start time
2020-11-07 13:25:39.057
End
2020-11-07 13:26:27.519
Duration
0:00:48.462
Note, WebLog generation is not included in the time.

CASA logs for stage 6